Thicknesses of mare basalts on the Moon from gravity and topography-Reference-Cited by-同舟云学术

Thicknesses of mare basalts on the Moon from gravity and topography

Published:2016-05 Issue:5 Volume:121 Page:854-870
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Gong Shengxia¹²,Wieczorek Mark A.²^ORCID,Nimmo Francis³,Kiefer Walter S.⁴,Head James W.⁵,Huang Chengli¹,Smith David E.⁶,Zuber Maria T.⁶

Affiliation:

1. Key Laboratory of Planetary Sciences, Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai China

2. Insitut de Physique du Globe de Paris, Sorbonne Paris Cité Université Paris Diderot Paris France

3. Department of Earth and Planetary Sciences University of California Santa Cruz California USA

4. Lunar and Planetary Institute Houston Texas USA

5. Department of Earth, Environmental and Planetary Sciences Brown University Providence Rhode Island USA

6. Department of Earth, Atmospheric, and Planetary Sciences Massachusetts Institute of Technology Cambridge Massachusetts USA

Funder

National Natural Science Foundation of China

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016JE005008

Reference59 articles.

1. Estimates of cryptomare thickness and volume in Schiller‐Schickard, Mare Humorum and Oceanus Procellarum areas;Antonenko I.;Proc. Lunar Planet. Sci. Conf.,1995

2. Evidence for basaltic volcanism on the Moon within the past 100 million years

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